V. V. Dyachenko
Russian Academy of Sciences
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Featured researches published by V. V. Dyachenko.
Nuclear Fusion | 2007
A. D. Gurchenko; E. Z. Gusakov; A. B. Altukhov; A. Yu. Stepanov; L. A. Esipov; M Yu Kantor; D. V. Kouprienko; V. V. Dyachenko; S. I. Lashkul
A fine scale drift wave mode possessing unusually high frequency 2?3?MHz and radial wave number is observed using the correlative upper hybrid resonance backscattering technique at the FT-2 tokamak under conditions when the ETG mode should be unstable. The radial wave number spectrum of turbulence is measured and shown to be maximal at values 120?170?cm?1 corresponding to the largest ETG instability growth rate.
Nuclear Fusion | 2011
V. K. Gusev; R.M. Aminov; A.A. Berezutskiy; V V Bulanin; F. V. Chernyshev; I. N. Chugunov; A.V. Dech; V. V. Dyachenko; A. E. Ivanov; S. A. Khitrov; N.A. Khromov; G. S. Kurskiev; M. M. Larionov; A.D. Melnik; V. B. Minaev; A.B. Mineev; M. I. Mironov; I.V. Miroshnikov; E. E. Mukhin; A.N. Novokhatsky; A. Panasenkov; M. I. Patrov; A V Petrov; Yu. V. Petrov; K.A. Podushnikova; V. Rozhansky; V.V. Rozhdestvensky; N. V. Sakharov; A.E. Shevelev; I. Yu. Senichenkov
The experimental and theoretical results obtained in the last two years on the interaction of neutral particle beams and high-frequency waves with a plasma using the spherical tokamak Globus-M are discussed. The experiments on the injection of low-energy proton beam of ~300 eV directed particle energy are performed with a plasma gun that produces a hydrogen plasma jet of density up to 3 × 1022 m−3 and a high velocity up to 250 km s−1. A moderate density rise (up to 30%) is achieved in the central plasma region without plasma disruption. Experiments on high-energy (up to 30 keV) neutral beam injection into the D-plasma are analysed. Modelling results on confinement of fast particles inside the plasma column that follows the neutral beam injection are discussed. The influence of the magnetic field on the fast particle losses is argued. A neutral beam injection regime with primary ion heating is obtained and discussed. The new regime with fast current ramp-up and early neutral beam injection shows electron temperature rise and formation of broad Te profiles until the q = 1 flux surface enters the plasma column. An energetic particle mode in the range of frequencies 5–30 kHz and toroidal Alfven eigenmodes in the range 50–300 kHz are recorded in that regime simultaneously with the Te rise. The energetic particle mode and toroidal Alfven eigenmodes behaviour are discussed. The toroidal Alfven eigenmode spectrum appears in Globus-M as a narrow band corresponding to n = 1. The first experimental results on plasma start-up and noninductive current drive generation are presented. The experiments are carried out with antennae providing mostly poloidal slowing down of waves with a frequency of 920 MHz, which is higher than a lower hybrid one existing under the experimental conditions. The high current drive efficiency is shown to be high (of about 0.25 A W−1), and its mechanism is proposed. Some near future plans of the experiments are also discussed.
Plasma Physics and Controlled Fusion | 2010
E. Z. Gusakov; V. V. Dyachenko; M A Irzak; S A Khitrov; A N Saveliev; O N Shcherbinin
The problem of lower hybrid (LH) wave excitation and current drive (CD) in tokamaks with a small aspect ratio (spherical tokamaks) is discussed. It is proposed to solve this problem by exciting the waves slowed down in the poloidal rather than the toroidal direction. As a result, due to the strong poloidal inhomogeneity of the magnetic field in spherical tokamaks, even the waves with comparatively weak slowing down (N ? 3?5) excited by a waveguide antenna in the equatorial plane can penetrate into the dense plasma and be absorbed via the Landau mechanism. This approach was applied for modeling the LHCD experiments in the low aspect ratio tokamak Globus-M (R = 0.36?m, a0 = 0.24?m, B0 = 0.4?T, Ip = 0.25?MA, vertical elongation k = 1.6, operating frequency 2.45?GHz). The modeling was carried out using four independent codes: (i) the self-consistent antenna coupling code GRILL3D, (ii) the ray-tracing code incorporating a specially developed ray-tracing technique including some corrections necessary in strongly inhomogeneous plasma, (iii) the 2D full-wave code WAVETOP2D and (iv) the Fokker?Plank code combined with the ray-tracing code allowing simulation of the driven current density profile. The results of simulations were cross-checked and appeared to be in a good agreement. It was demonstrated that the proposed scenario provides a possibility for the efficient LHCD in a spherical tokamak.
Monthly Notices of the Royal Astronomical Society | 2016
Artem Y. Burdanov; Paul Benni; V. Krushinsky; A. Popov; Evgenii N. Sokov; Iraida A. Sokova; Sergei A. Rusov; Artem Yu. Lyashenko; K. Ivanov; A. V. Moiseev; Denis A. Rastegaev; V. V. Dyachenko; Y.Y. Balega; Ö. Baştürk; I. Özavcı; Damian Puchalski; Alessandro Marchini; Ramon Naves; Stan Shadick; Marc Bretton
We present the first results of our search for transiting exoplanet candidates as part of the Kourovka Planet Search (KPS) project. The primary objective of the project is to search for new hot Jupiters which transit their host stars, mainly in the Galactic plane, in the
Plasma Physics and Controlled Fusion | 2000
S. I. Lashkul; V. N. Budnikov; A A Borevich; E O Chechik; V. V. Dyachenko; P R Goncharov; L. A. Esipov; E. R. Its; M Yu Kantor; D. V. Kouprienko; A. Yu. Popov; K. A. Podushnikova; I E Sackharov; S. V. Shatalin; V B Yermolaev
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Monthly Notices of the Royal Astronomical Society | 2016
O.V. Maryeva; E. L. Chentsov; V.P. Goranskij; V. V. Dyachenko; S.V. Karpov; E. V. Malogolovets; Denis A. Rastegaev
magnitude range of 11 to 14 mag. Our observations were performed with the telescope of the MASTER robotic network, installed at the Kourovka astronomical observatory of the Ural Federal University (Russia), and the Rowe-Ackermann Schmidt Astrograph, installed at the private Acton Sky Portal Observatory (USA). As test observations, we observed three celestial fields of size
Nuclear Fusion | 2006
O. N. Shcherbinin; F. V. Chernyshev; V. V. Dyachenko; V. K. Gusev; Yu. V. Petrov; N. V. Sakharov; V.M. Leonov
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Nuclear Fusion | 2015
S. I. Lashkul; A. B. Altukhov; A. D. Gurchenko; E. Z. Gusakov; V. V. Dyachenko; L. A. Esipov; M. A. Irzak; M Yu Kantor; D. V. Kouprienko; A.A. Perevalov; A. N. Saveliev; S. V. Shatalin; A. Yu. Stepanov
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Czechoslovak Journal of Physics | 2002
S. I. Lashkul; V. N. Budnikov; A. D. Gurchenko; E. Z. Gusakov; V. V. Dyachenko; L. A. Esipov; E. R. Its; M Yu Kantor; D. V. Kouprienko; K. M. Novik; A. Yu. Popov; V. L. Selenin; A. Yu. Stepanov; V. B. Yermolajev; S. V. Shatalin; E. O. Vekshina
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Nuclear Fusion | 2015
V. V. Dyachenko; O. N. Shcherbinin; E. Z. Gusakov; V. K. Gusev; M A Irzak; G.S. Kurskiev; Yu. V. Petrov; A. N. Saveliev; N. V. Sakharov; S. A. Khitrov; N. A. Khromov; V. I. Varfolomeev; A. V. Voronin
during the period from 2012 to 2015. As a result, we discovered four transiting exoplanet candidates among the 39000 stars of the input catalogue. In this paper, we provide the description of the project and analyse additional photometric, spectral, and speckle interferometric observations of the discovered transiting exoplanet candidates. Three of the four transiting exoplanet candidates are most likely astrophysical false positives, while the nature of the fourth (most promising) candidate remains to be ascertained. Also, we propose an alternative observing strategy that could increase the projects exoplanet haul.